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- Centre National de la Recherche ScientifiqueFR339 papers
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- Max Planck Institute for AstronomyDE217 papers
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114 papers · 1 filter
The infrared counterpart and proper motion of magnetar SGR0501+4516
A. A. Chrimes, A. J. Levan, J. D. Lyman +19
Soft gamma repeaters (SGRs) are highly magnetised neutron stars (magnetars) notable for their gamma-ray and X-ray outbursts. In this paper, we use near-infrared (NIR) imaging of SG…
ATCA Study of Small Magellanic Cloud Supernova Remnant 1E 0102.2-7219
Rami Z. E. Alsaberi, M. D. Filipović, S. Dai +29
We present new and archival Australia Telescope Compact Array and Atacama Large Millimeter/submillimeter Array data of the Small Magellanic Cloud supernova remnant 1E 0102.2-7219 a…
Type Ia Supernova Nucleosynthesis: Metallicity-Dependent Yields
James D Keegans, Marco Pignatari, Richard J Stancliffe +7
Type Ia supernova explosions (SNIa) are fundamental sources of elements for the chemical evolution of galaxies. They efficiently produce intermediate-mass (with Z between 11 and 20…
New ASKAP Radio Supernova Remnants and Candidates in the Large Magellanic Cloud
Luke M. Bozzetto, Miroslav D. Filipović, H. Sano +34
We present a new Australian Square Kilometre Array Pathfinder (ASKAP) sample of 14 radio Supernova Remnant (SNR) candidates in the Large Magellanic Cloud (LMC). This new sample is…
A New Emulated Monte Carlo Radiative Transfer Disk-Wind Model: X-Ray Accretion Disk-wind Emulator -- XRADE
G. A. Matzeu, M. Lieu, M. T. Costa +14
We present a new X-Ray Accretion Disk-wind Emulator (\textsc{xrade}) based on the 2.5D Monte Carlo radiative transfer code which provides a physically-motivated, self-consistent tr…
Origins of the UV/X-ray Relation in Arakelian 120
Ra'ad David Mahmoud, Chris Done, Delphine Porquet +1
We explore the accretion geometry in Arakelian 120 using intensive UV and X-ray monitoring from \textit{Swift}. The hard X-rays ( keV) show large amplitude, fast (few-day) va…